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The perihelion advance according to a post-NEWTONian gravitational law with logarithmic correction term

✍ Scribed by J. P. Mücket; H.-J. Treder


Publisher
John Wiley and Sons
Year
1977
Tongue
English
Weight
145 KB
Volume
298
Category
Article
ISSN
0004-6337

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✦ Synopsis


Abstract

By a gravitational potential Φ′(r) = − G~0~M/r (I + α + α In r) with |α|≪ 1 a motion δφ of the perihelion of a planet is resulting which is neither depending on the central‐mass M nor on the semi‐axis of the KEPLER‐ellipse δφ ≈︁ ‐ απ. Therefore, |α| must be smaller than 10^−8^.